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Posted: Dec 21, 2017
'Cosmic lantern' could help us further understand the fate of the universe
(Nanowerk News) New research has provided a deeper insight into emission line galaxies, used in several ongoing and upcoming surveys, to help us further understand the composition and fate of the Universe.
The quest to determine the nature of both dark matter and dark energy has led scientists to adopt new tracers of the large-scale structure of the Universe, such as emission line galaxies. These galaxies present strong emission lines from the gas heated up by newly formed stars.
The image shows a slice of a numerical model for dark matter (grey points) and galaxies. Two types of galaxies are shown: bright emission line galaxies (filled circles) and those galaxies hosted by gravitational potentials above a threshold such that the number density equals that of the emission line galaxies (open circles). This figure illustrates that emission line galaxies trace different features from the cosmic web than galaxies selected by either their stellar mass or the strength of the gravitational potential where they have formed. (Image: University of Portsmouth)
Lead author of the study (Monthly Notices of the Royal Astronomical Society, "The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5"), Dr Violeta Gonzalez-Perez from the University of Portsmouth’s Institute of Cosmology and Gravitation, said: “Galaxies are cosmic lanterns that show small patches of cosmic history, informing us of the changes in the space-time fabric of the Universe. The strong formation of new stars in galaxies leave a characteristic imprint in their spectra that allows for a precise determination of their distance.
“Moreover, as young stars are very bright, galaxies with a strong star formation can be visible further back in cosmic time. These are the two characteristics that make emission line galaxies excellent cosmological tracers for a long time span.”
However, current emission line galaxy samples are small and their characteristics are not well understood. Computational modelling is the only way to attempt to understand all the processes involved in the formation and evolution of these galaxies.
The image shows the location of some the emission line galaxies observed in the study (green circles) against the images of a big patch of the sky as observed by The Dark Energy Camera Legacy Survey (DECaLS) http://legacysurvey.org/decamls/. (Image: University of Portsmouth)
Astronomers from the University of Portsmouth’s world-leading Institute of Cosmology and Gravitation (ICG) explored the characteristics of emission line galaxies through experiments on DiRAC's (Distributed Research utilising Advanced Computing) national supercomputing facility at Durham University.
The computational experiments were concentrated around the time when the Universe went from being matter dominated to becoming dark energy dominated as it is now. They found that most emission line galaxies live at the centres of gravitational potential wells, with masses equivalent to eleven billion of our suns. Current numerical models of formation and evolution of galaxies also show that emission line galaxies trace the underlying gravitational potentials in a different way to galaxies selected by their stellar mass.
They then compared their results with the expectations from the SDSS-IV/eBOSS surveys and Dark Energy Spectroscopic Instrument (DESI). Both surveys aim to measure the effect of dark energy on the expansion of the Universe.
Dr Gonzalez-Perez said: “This comparison will improve our understanding of galaxy formation and evolution and allow scientists to benefit from a more realistic model for the mechanisms that produce emission line galaxies.”
The image shows nearby emission line galaxies NCG 4038 - 4039. The pink parts in this image are showing the light from the gas heated by newly formed stars. (Image: NASA, ESA and The Hubble Heritage (STScl/AURA)-ESA/Hubble Collaboration)
Next summer, the SDSS-IV/eBOSS survey is expected to have the first cosmological results from these tracers. In the coming years, the Dark Energy Survey Instrument (DESI) will expand this usage of emission line galaxies as cosmological tracers. The DESI will see their first light in 2019 and it will measure the spectra of 35 million galaxies, which is eight times more than the current SDSS has proved. In 2021, Euclid will start collecting spectra for 50 million sources, solely focusing on emission line galaxies. The ICG is involved in both surveys.